How is it that we can get clear photos of distant galaxies and nebulas, but any shot of Pluto is a blur?
Galaxies occupy more area in the sky. Their angular size is much more than planets.
The angular diameter of Andromeda galaxy is about 3 degree Moon is about 30 arc minute( or half degree)...Where as Pluto varies from 0.0608 arc seconds to 0.116 arc seconds.
3600 arc seconds = one degree.
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Distant galaxies and nebulas are captured with powerful telescopes, while Pluto, being in our solar system, is imaged from a much closer range, making its details harder to discern. Additionally, Pluto's small size and distance contribute to the challenges in obtaining clear images.
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The clarity of astronomical images, whether of distant galaxies and nebulas or of objects within our solar system like Pluto, depends on several factors:
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Distance: Distant galaxies and nebulae are typically much larger and emit more light than individual objects within our solar system. This makes them easier to capture with telescopes, even from great distances.
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Light Gathering Power: Telescopes used for observing distant galaxies and nebulae are often large and equipped with powerful optics that can gather and focus light effectively. This enables them to capture detailed images even from very faint sources.
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Resolution: Distant galaxies and nebulae are composed of numerous stars, gas clouds, and other structures, which can be resolved by telescopes with high resolution capabilities. Advanced imaging techniques and longer exposure times can further enhance the resolution of these images.
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Motion and Atmosphere: Objects within our solar system, such as Pluto, are much closer and often move relative to Earth at a faster pace. Additionally, Earth's atmosphere can distort and blur images of objects at such distances. Achieving clear images of objects within our solar system requires compensating for their motion and minimizing atmospheric interference, which can be challenging.
In summary, clear images of distant galaxies and nebulae are achievable due to their size, light emission, and the capabilities of advanced telescopes. On the other hand, capturing clear images of objects within our solar system, like Pluto, presents challenges related to their smaller size, motion, and atmospheric interference.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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